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NASA NTRS ยท 20060036731

Evolving Magnetic Structures and Their Relation to Coronal Mass Ejections

Abstract

Solar activity regions are frequently concentrated into cluster which persist for many solar rotations. These activity complexes are associated with weak dispersed magnetic fields which are most apparent after the activity itself has ceased. We call this combination of persistent activity and dispersed Evolving Magnetic Structures (EMS). Here we show examples of EMSs and describe the evolution of an EMS associated with major Coronal Mass Ejections (CME) and other solar and magnetic disturbances.

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BibTeXRIS

Feynman, J.. 1996-01-01. Evolving Magnetic Structures and Their Relation to Coronal Mass Ejections. https://ntrs.nasa.gov/citations/20060036731

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